Solid CO Spectroscopy: Embedded YSOs in Taurus-Auriga

Details Solid CO Spectroscopy: Embedded YSOs in Taurus-Auriga Solid CO Spectroscopy: Embedded YSOs in Taurus-Auriga

Feb 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.224..573t&link_type=abstract

Astrophysics and Space Science, Volume 224, Issue 1-2, pp. 573-574

Astronomy and Astrophysics

Astrophysics

Grain Mantles, Infrared:Ism:Lines And Bands, Stars: Pre-Main-Sequence

Scientific paper

Infrared spectra of the 4.67µm solid CO feature were obtained for YSOs in Taurus. A first attempt is made to analyse the likely composition of the CO ices. Column densities are derived from the spectra, and compared with the ones predicted for a low mass protostar. The strengths of the CO- and water-ice features towards those objects are compared.

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